Read this response and predict the preceding dialog. Neutrinos are also released by the fusion reactions in the core, but unlike photons they very rarely interact with matter, so almost all are able to escape the Sun immediately.

Convo:
Anonymous A) What is the approximate time scale of the solar core?;
Anonymous B) According to current models, random scattering from free electrons in the solar radiative zone (the zone within 75% of the solar radius, where heat transfer is by radiation) sets the photon diffusion time scale (or "photon travel time") from the core to the outer edge of the radiative zone at about 170,000 years.;
Anonymous A) Are there any other interesting aspects about this article?;
Anonymous B) From there they cross into the convective zone (the remaining 25% of distance from the Sun's center), where the dominant transfer process changes to convection, and the speed at which heat moves outward becomes considerably faster.;
Anonymous A) What is the significance of the solar core?;
Anonymous B) In the process of heat transfer from core to photosphere, each gamma ray in the Sun's core is converted during scattering into several million visible light photons before escaping into space.;
Anonymous A) What else does the solar core contribute to the atmosphere?;
Anonymous B) 